26 Fe 55.845

Iron

Transition metal Ferrum solid

[Ar] 3d⁶ 4s² · 2 · 8 · 14 · 2

The metal that named an age and makes up the core of our planet. Iron is the cheapest and most-produced structural material in history, and it is also what carries oxygen in the blood of every vertebrate.

3D model

Bohr model: nucleus and electron shells from the real configuration. Valence electrons are highlighted.

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Atomic properties

Atomic number
26
Atomic mass
55.845 а.е.м.
№93 / 118
Electron configuration
[Ar] 3d⁶ 4s²
Electrons per shell
2 · 8 · 14 · 2
Block
d-block
Group
Iron group
Period
4
Electronegativity (Pauling)
1.83
№42 / 100
Electronegativity (Allen)
1.8
Atomic radius
156 pm
№67 / 103
Covalent radius
132 pm
№89 / 118
Van der Waals radius
194 pm
Ionisation energy 1
762.5 kJ/mol
№41 / 118
Ionisation energy 2
1 561.9 kJ/mol
Ionisation energy 3
2 957 kJ/mol
Ionisation energy 4
5 290 kJ/mol
Ionisation energy 5
7 240 kJ/mol
Electron affinity
15.7 kJ/mol
№81 / 108
Common oxidation states
+2, +3
Oxidation states
-4, -2, -1, +1, +2, +3, +4, +5, +6, +7

Physical properties

State at 25 °C
solid
Density
7.874 g/cm³
№60 / 118
Melting point
1 811 K · 1 537.9 °C
№27 / 111
Boiling point
3 134 K · 2 860.9 °C
№40 / 107
Speed of sound
5 120 m/s
№12 / 72

Thermal properties

Heat of fusion
13.81 kJ/mol
№38 / 98
Heat of vaporisation
340 kJ/mol
№32 / 98
Specific heat capacity
0.449 J/(g·K)
№27 / 95
Thermal conductivity
80.4 W/(m·K)
№25 / 96

Mechanical properties

Young's modulus
211 GPa
№12 / 70
Shear modulus
82 GPa
Bulk modulus
170 GPa
Poisson ratio
0.29
Mohs hardness
4
№25 / 57
Brinell hardness
490 MPa

Electrical and magnetic properties

Electrical resistivity
96.1 nΩ·m
№63 / 84
Magnetic ordering
ferromagnetic
Curie point
1 043 K
Néel point
no data
Superconducting point
no data

Crystal structure

Crystal structure
body-centred cubic (bcc)
Lattice constants
a = 286.65 pm

Abundance

In the crust
56 300 mg/kg
№4 / 88
In the ocean
0.002 mg/L
№28 / 78
In the universe
1.1·10⁶ mg/kg
№6 / 83
In the human body
60 mg/kg
№13 / 40

Isotopes

Isotope Abundance Half-life Decay mode
54Fe 5.845 % stable
56Fe 91.754 % stable
57Fe 2.119 % stable
58Fe 0.282 % stable
60Fe 2.6 Myr β−

Iron-56 has the highest binding energy per nucleon of any nucleus: past it neither fusion nor fission releases energy, which is why stellar burning ends at iron.

Discovery

Year of discovery
known since antiquity
Discovered by
known since antiquity
Where
no data
Origin of the name
Old English iren; the symbol Fe is from Latin ferrum

History

The first iron people used was meteoritic; the Egyptians called it metal from the sky. Smelting from ore began around 1200 BCE in Anatolia and displaced bronze within a few centuries — not because iron is better, but because its ores are incomparably more common.

Where it occurs

The fourth most abundant element in the crust at 5.6 %, and the most abundant in the whole Earth once you count the core. The main ores are haematite and magnetite; the largest deposits formed 2.4 billion years ago when new oxygen precipitated the iron dissolved in the oceans.

How it is produced

The blast furnace: ore, coke and limestone give pig iron, which is then blown with oxygen in a converter to burn off excess carbon. Direct reduction with hydrogen is the route to carbon-free steelmaking.

Role in living things

Haemoglobin: one iron atom in a haem binds one oxygen molecule, and four haems per protein carry oxygen from lungs to tissue. Iron deficiency is the most common nutritional deficiency in the world.

Safety

Iron itself is harmless, but acute poisoning from iron supplements is a frequent cause of childhood poisoning. Hereditary haemochromatosis lets iron accumulate and damages the liver and heart.

Uses

  • Steel: over 95 % of all metal produced worldwide by mass
  • Cast iron for castings and machine beds
  • Magnetic cores for transformers and motors
  • The catalyst in Haber–Bosch ammonia synthesis
  • Pigments: ochre, red lead oxide, iron oxide reds

Curiosities

  • The iron-56 nucleus sits at the bottom of the energy curve — which is precisely why massive stars explode once they reach iron.
  • Iron's Curie point is 1043 K: above it a magnet stops being a magnet.
  • Blood is red and mollusc haemolymph is blue because they carry oxygen on copper rather than iron.
  • Meteoritic iron was worked two thousand years before smelting began: the dagger from Tutankhamun's tomb is made of it.
  • Earth's magnetic field is generated by convecting liquid iron in the outer core.

Position in the table

Fe